Generally speaking, IR emission from young shell-type SNRs only shows up in emission from the shell of the remnant. This emission results from warmed interstellar grains; searches for dust associated with the ejecta in SNRs has turned up very little [1]}, [2]}. As an example, in Figure REF , we show the IR emission from DEM L71, the remnant whose X-ray emission is shown in Figure REF .
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